Ertan, Ünal and Alpar, M. Ali (2021) The minimum rotation period of millisecond pulsars. Monthly Notices of the Royal Astronomical Society: Letters, 505 (1). L112-L114. ISSN 1745-3925 (Print) 1745-3933 (Online)
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Official URL: http://dx.doi.org/10.1093/mnrasl/slab060
Abstract
A simple and natural explanation for the minimum period of millisecond pulsars follows from a correlation between the accretion rate and the frozen surface dipole magnetic field resulting from ohmic diffusion through the neutron star crust in initial stages of accretion in low-mass X-ray binaries.
| Item Type: | Article |
|---|---|
| Divisions: | Faculty of Engineering and Natural Sciences > Basic Sciences > Physics Faculty of Engineering and Natural Sciences |
| Depositing User: | Ünal Ertan |
| Date Deposited: | 24 Nov 2021 15:20 |
| Last Modified: | 25 Aug 2022 20:50 |
| URI: | https://research.sabanciuniv.edu/id/eprint/42559 |
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